Document Type


Publication Date



We report on a search for continuous gravitational wave emission from three recycled radio pulsars, performed by using the data of the resonant detector AURIGA. Given the spin rate of the selected targets – the isolated pulsar PSR J1939+2134 and the binary pulsars PSR J0024-7204J and PSR J0218+4232 – the expected frequency of the emitted gravitational waves falls in the high sensitivity range of the detector.

Source Citation

A. Mion, ., M. J. Benacquista, ., M. Kramer, ., P. P. C. Freire, ., & A. Possenti, .(2009). A Search For Periodic Gravitational Waves From Three Recycled Pulsars Using The Auriga Detector - An Implementation Of A Modified Version Of The Unified Approach Method. Astronomy And Astrophysics, 504(2), 673-679.



To view the content in your browser, please download Adobe Reader or, alternately,
you may Download the file to your hard drive.

NOTE: The latest versions of Adobe Reader do not support viewing PDF files within Firefox on Mac OS and if you are using a modern (Intel) Mac, there is no official plugin for viewing PDF files within the browser window.